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• W2047378894 abstract "Dark matter with Sommerfeld-enhanced annihilation has been proposed to explain observed cosmic ray positron excesses in the 10 GeV to TeV energy range. We show that the required enhancement implies thermal relic densities that are too small to be all of dark matter. We also show that the dark matter is sufficiently self-interacting that observations of elliptical galactic dark matter halos exclude large Sommerfeld enhancement for light force carriers. Resonant Sommerfeld enhancement does not modify these conclusions, and the astrophysical boosts required to resolve these discrepancies are disfavored, especially when significant self-interactions suppress halo substructure." @default.
• W2047378894 created "2016-06-24" @default.
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• W2047378894 date "2010-04-15" @default.
• W2047378894 modified "2023-10-12" @default.
• W2047378894 title "Halo-Shape and Relic-Density Exclusions of Sommerfeld-Enhanced Dark Matter Explanations of Cosmic Ray Excesses" @default.
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• W2047378894 doi "https://doi.org/10.1103/physrevlett.104.151301" @default.
• W2047378894 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/20481979" @default.
• W2047378894 hasPublicationYear "2010" @default.
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